These headlines accompanied the announcement of a candidate SETI signal by a team of scientists using a telescope located in Russia. For those who like difficult-to-remember names, the telescope is the RATAN-600 radio telescope in Zelenchukskaya, in the Karachay-Cherkess Republic of Russia. While no official scientific publications accompanied the announcement, the results will be presented at an international conference in Mexico in late September 2016. Given all the hype surrounding the “signal,” I thought it worthwhile to provide some perspective.

What They Claim

On May 15, 2015, the RATAN-600 telescope observed a signal at 11 GHz with an amplitude of 0.75 Janskys. While not a particularly strong signal, it is well above background noise. The configuration of the RATAN-600 telescope results in an unusual beam on the sky (highly elongated in the north-south direction), making a precise location difficult to determine. However, the signal is consistent with the direction of a star called HD 164595. Some images of the data have circulated around the Internet (since the official data has not yet been published). As the example below shows, the signal lasted for a couple of seconds and is well above background noise.

Image: Strong signal from the direction of HD 164595. “Raw” record of the signal together with expected shape of the signal for point-like source in the position of HD 164595. Credit: Bursov et al.

Why It Is Interesting

HD 164595 is a star with similar characteristics to the Sun. It has an estimated age of 6.3 billion years (4.6 billion for the Sun) and 99 percent the mass of the Sun. The metallicity of HD 164595 matches the Sun’s, and the star hosts a Neptune-sized planet orbiting with a period of 40 days (Mercury takes 88 days to complete one revolution). The dynamics of the exoplanet allow for other exoplanets around the star although none have been detected yet. A distance of 94 light-years makes HD 164595 a next-door neighbor in astronomical terms—the center of the Milky Way galaxy resides 25,000 light-years away.

If the signal detected by the RATAN-600 telescope originates from a planet or moon orbiting HD 164595, then the proximity of the star means that we can investigate it in much more detail over the next couple of decades as our planet-finding technology increases. Even our current technology would allow sending a probe that would reach the planet in a few centuries.

Reasons to Doubt Aliens Exist

First, according to the Space.com article, the team observed the direction of HD 164595 nearly 40 times and only detected the signal on one of the observations. While it’s possible that some alien civilization turned on a beacon for just a short period that the team happened to detect, the lack of reproducibility makes a more mundane explanation probable. This measurement will likely join the Wow! signal and the Valentine’s Day monopole on the list of results that scientists can never fully explain.

Second, assuming the signal does originate from HD 164595, astronomers can estimate the amount of power required to generate such a signal. A civilization beaming the signal toward Earth would require more than a trillion watts of power to accomplish the task. Collectively, the world’s population uses (on average) about 10 trillion watts of energy, so this alien civilization would have had to harness at least one-tenth of the world’s energy. If no beaming occurred and the signal went out isotropically into the galaxy, it would require hundreds of times more energy than the surface of the Earth receives from the Sun! Wait a second—maybe this explains why the signal lasted for such a short period of time.

Third, the characteristics of the RATAN-600 telescope introduce some ambiguity regarding the nature of the measurement. The unusual beam pattern of the telescope is consistent with the location of HD 164595, but by no means demands that the signal originates from that direction. Also, normal SETI searches utilize a much narrower frequency band (roughly 1 billion times narrower). The wide bandwidth of RATAN-600 greatly increases the possible explanations of the measured signal.

Even SETI astronomers are skeptical that the signal represents communication from aliens as they monitor the region with the Allen Telescope Array. Nothing yet, but I’ll keep you informed of anything new.

About The Author

Since my earliest memories, science and the Christian faith have featured prominently in my life - but I struggled when my scientific studies seemed to collide with my early biblical training. My first contact with RTB came when I heard Hugh Ross speak at Iowa State University. It was the first time I realized it was possible to do professional work incorporating both my love of science and my desire to serve God. I knew RTB's ministry was something I was called to be a part of.
While many Christians and non-Christians see the two as in perpetual conflict, I find they integrate well. They operate by the same principles and are committed to discovering foundational truths. My passion at RTB is helping Christians see how powerful a tool science is to declare God's glory and helping scientists understand how the established scientific discoveries demonstrate the legitimacy and rationality of the Christian faith.
While many Christians and non-Christians see the two as in perpetual conflict, I find they integrate well.
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Jeff Zweerink thought he would follow in his father's footsteps as a chemistry professor until a high school teacher piqued his interest in physics. Jeff pursued a BS in physics and a PhD in astrophysics at Iowa State University (ISU), where he focused his study on gamma rays - messengers from distant black holes and neutron stars.
Upon completing his education, Jeff taught at Loras College in Dubuque, Iowa. Postdoctoral research took him to the West Coast, to the University of California, Riverside, and eventually to a research faculty position at UCLA. He has conducted research using STACEE and VERITAS gamma-ray telescopes, and currently works on GAPS, a balloon experiment seeking to detect dark matter.
A Christian from childhood, Jeff desired to understand how the worlds of science and Scripture integrate. He struggled when his scientific studies seemed to collide with his early biblical training. While an undergrad at ISU, Jeff heard Hugh Ross speak and learned of Reasons to Believe (RTB) and its ministry of reconciliation - tearing down the presumed barriers between science and faith and introducing people to their personal Creator. Jeff knew this was something he was called to be a part of.
Today, as a research scholar at RTB, Jeff speaks at churches, youth groups, universities, and professional groups around the country, encouraging people to consider the truth of Scripture and how it connects with the evidence of science. His involvement with RTB grows from an enthusiasm for helping others bridge the perceived science-faith gap. He seeks to assist others in avoiding the difficulties he experienced.
Jeff is author of Who's Afraid of the Multiverse? and coauthor of more than 30 journal articles, as well as numerous conference proceedings. He still serves part-time on the physics and astronomy research faculty at UCLA. He directs RTB's online learning programs, Reasons Institute and Reasons Academy, and also contributes to the ministry's podcasts and daily blog, Today's New Reason to Believe.
When he isn’t participating in science-faith apologetics Jeff enjoys fishing, camping, and working on home improvement projects. An enthusiastic sports fan, he coaches his children's teams and challenges his RTB colleagues in fantasy football. He roots for the Kansas City Chiefs and for NASCAR's Ryan Newman and Jeff Gordon. Jeff and his wife, Lisa, live in Southern California with their five children.